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Redundant versus non-redundant apertures for exoplanet detection

Published online by Cambridge University Press:  28 May 2003

C. Aime
Affiliation:
UMR 6525 Astrophysique, University of Nice Sophia-Antipolis, 06108 Nice Cedex 2, France
R. Soummer
Affiliation:
UMR 6525 Astrophysique, University of Nice Sophia-Antipolis, 06108 Nice Cedex 2, France
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Abstract

Using simplificative assumptions, we show that a redundant configuration of diluted apertures should permit an easier exoplanet detection than a non-redundant one. This result assumes that after coronagraphy the planet appears over an uniform background whose statistical fluctuation is the unique source of noise. The detection is made using a matched filter, cross-correlating the observed image with the telescope array PSF. In that case, the relevant parameter appears to be the integral of the modulus squared of the aperture MTF.

Type
Research Article
Copyright
© EAS, EDP Sciences, 2003

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